Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A cosmological view of extreme mass-ratio inspirals in nuclear star clusters
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1205.2702.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
32
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 1bd11613-3f59-494d-bd18-ffb79af45f53 · inbound
Assessing EMRI Detectability of the Rotating Quantum Oppenheimer-Snyder Black Hole cites this paper.
Assessing EMRI Detectability of the Rotating Quantum Oppenheimer-Snyder Black Hole A cosmological view of extreme mass-ratio inspirals in nuclear star clusters
Reference 45
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T20:51:10.093187Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 2fab6648-7ed2-497e-ac9f-0c47476fa15c · inbound
Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations cites this paper.
Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations A cosmological view of extreme mass-ratio inspirals in nuclear star clusters
Reference 68
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T01:01:27.051529Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.